NASA NTRS · 19830016069
Dynamic alignment and selective decay in MHD
Abstract
Under some circumstances, incompressible magnetohydrodynamic turbulence will evolve toward a state in which the velocity fields and magnetic fields are aligned or anti-aligned. We propose a mechanism for this effect and illustrate with numerical computations. Under some other circumstances, the energy appears to decay selectively toward a minimum energy state in which the kinetic energy has disappeared. It has not been possible so far to identify a boundary in the phase space which divides the two regimes.
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Matthaeus, W. H., Montgomery, D.. 1983-01-01. Dynamic alignment and selective decay in MHD. https://ntrs.nasa.gov/citations/19830016069
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